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Proceedings Paper

Twilight ray height determination
Author(s): L. S. Shakun; V. D. Motritch
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Paper Abstract

A new program that simulates the primary light dispersion in atmosphere during twilight is represented. Program uses the modified N. B. Divari model of light dispersion in the atmosphere. Optical depths, the twilight beam height and its half-width may be easily and with high speed obtained using this program. The flexible program construction may be used for the determination the twilight beam parameters by iteration. Obtained results coincide with those in literature.

Paper Details

Date Published: 3 September 1997
PDF: 5 pages
Proc. SPIE 3237, 23rd European Meeting on Atmospheric Studies by Optical Methods, (3 September 1997); doi: 10.1117/12.284778
Show Author Affiliations
L. S. Shakun, Odessa State Univ. (Ukraine)
V. D. Motritch, Odessa State Univ. (Ukraine)


Published in SPIE Proceedings Vol. 3237:
23rd European Meeting on Atmospheric Studies by Optical Methods
Vasily N. Ivchenko, Editor(s)

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